Bosonic Quantum Computational Complexity

TL;DR

This paper develops a foundational quantum complexity theory for bosonic systems with infinite-dimensional Hilbert spaces, introducing new classes, problems, and analyzing their computational properties.

Contribution

It establishes a formal framework for bosonic quantum complexity, defining classes, problems, and exploring their relationships and computational bounds.

Findings

Quadratic (Gaussian) quantum dynamics are equivalent to class BQL.

Deciding the spectrum boundedness of bosonic Hamiltonians is co-NP-hard.

Minimum energy computation depends on the non-Gaussian stellar rank, with complexity varying accordingly.

Abstract

Quantum computing involving physical systems with continuous degrees of freedom, such as the quantum states of light, has recently attracted significant interest. However, a well-defined quantum complexity theory for these bosonic computations over infinite-dimensional Hilbert spaces is missing. In this work, we lay foundations for such a research program. We introduce natural complexity classes and problems based on bosonic generalizations of BQP, the local Hamiltonian problem, and QMA. We uncover several relationships and subtle differences between standard Boolean classical and discrete variable quantum complexity classes and identify outstanding open problems. In particular: 1. We show that the power of quadratic (Gaussian) quantum dynamics is equivalent to the class BQL. More generally, we define classes of continuous-variable quantum polynomial time computations with a bounded probability of error based on higher-degree gates. Due to the infinite dimensional Hilbert space, it is not a priori clear whether a decidable upper bound can be obtained for these classes. We identify complete problems for these classes and demonstrate a BQP lower and EXPSPACE upper bound. We further show that the problem of computing expectation values of polynomial bosonic observables is in PSPACE. 2. We prove that the problem of deciding the boundedness of the spectrum of a bosonic Hamiltonian is co-NP-hard. Furthermore, we show that the problem of finding the minimum energy of a bosonic Hamiltonian critically depends on the non-Gaussian stellar rank of the family of energy-constrained states one optimizes over: for constant stellar rank, it is NP-complete; for polynomially-bounded rank, it is in QMA; for unbounded rank, it is undecidable.